View allAll Photos Tagged planetary

Swimming with a pod of elders during one of our Wild Dolphin Retreats

Cresent moon with venus and jupiter

Sweet graffiti outside the hostel I stayed at, Sleeping in Heaven in Norrebro, Copenhagen.

Spindle for the largest truck on earth.

Usados en los camiones removedores de tierra mas grandes del mundo

 

Prometheus dips into the inner F ring at its farthest point from Saturn in

its orbit, creating a dark gore and a corresponding bright streamer. Gores

created during previous apoapsis (the name for the farthest point in an

orbit) passes, are seen above. The older gores are farther behind the moon

in its orbit of Saturn.

  

This view looks toward the unlit side of the rings from about 31 degrees

above the ringplane. Prometheus is 102 kilometers (63 miles) across.

  

The image was taken in visible light with the Cassini spacecraft

narrow-angle camera on Nov. 1, 2006 at a distance of approximately 1.7

million kilometers (1.1 million miles) from Saturn and at a

Sun-Saturn-spacecraft, or phase, angle of 162 degrees. Image scale is 10

kilometers (6 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

  

credit: NASA/JPL/Space Science Institute

TEDxBoston Planetary Stewardship — November 13-14, Boston and Cambridge

Simple Planetary gears - www.thingiverse.com/thing:16897

    

Printed out perfectly, gears mesh so well! Very fun little toy to play with, but also a great demonstration of how you can actually print very usable gears with 3D printing!

 

The Cassini spacecraft looks toward daybreak on Saturn through the

delicate strands of the C ring. Some structure and contrast is visible in

the clouds far below.

  

This view looks toward the unlit side of the rings from about 18 degrees

above the ringplane.

  

The image was taken with the Cassini spacecraft narrow-angle camera using

a spectral filter sensitive to wavelengths of infrared light centered at

862 nanometers. The view was acquired on Nov. 4, 2006 at a distance of

approximately 1.7 million kilometers (1 million miles) from Saturn and at

a Sun-Saturn-spacecraft, or phase, angle of 162 degrees. Image scale is 10

kilometers (6 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

  

credit: NASA/JPL/Space Science Institute

Hen's egg backlit with red flash

 

Looking down through the A ring and Cassini Division, the Cassini spacecraft sees the

bright limb of Saturn. The view shows a portion the rings from the outer B ring, at upper

right, to the F ring at bottom.

  

See PIA08389 for a labeled map of Saturn's rings.

  

The perspective is toward the unilluminated side of the rings from about 15 degrees

above the ringplane.

  

The image was taken in visible light with the Cassini spacecraft narrow-angle camera

on Dec. 12, 2007. The view was acquired at a distance of approximately 2.2 million

kilometers (1.4 million miles) from Saturn. Image scale is 28 kilometers (17 miles)

per pixel in the radial, or outward from Saturn, direction; and 13 kilometers (8 miles)

per pixel in the longitudinal, or around Saturn, direction.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European Space

Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the

California Institute of Technology in Pasadena, manages the mission for NASA's

Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard

cameras were designed, developed and assembled at JPL. The imaging operations

center is based at the Space Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov.

The Cassini imaging team homepage is at ciclops.org .

 

credit: NASA/JPL/Space Science Institute

KILKENNY - Monday, 2nd November 2015 - The annual Science Foundation Ireland Science Summit begins today in Kilkenny. Taking place over two-days (2th-3th November) with the theme For Whats Next, the summit provides a platform for 300 members of Irelands research community to discuss Irelands science policy, programmes and progress. The summit will feature keynote speakers including Mr Chris Lewicki, President and Chief Engineer at Planetary Resources, a USA based asteroid mining company whose vision is to do the impossible now by developing a space economy through Asteroid mining.

This one-day symposium looks at the future. Intersections and The Arts Catalyst bring together an exceptional range of artists, academics and other industry experts to look at future approaches to living. It explored the possibility of creating new autonomous infrastructures across energy, trade and transport, offering a space for everyone to contribute to an active dialogue about our futures. Confirmed speakers include: expert on utopias Dr Malcolm Miles and international artists Lise Autogena, HeHe, London Fieldworks and Kate Rich.

 

Following the symposium, AV Festival 10 and BALTIC presented a free lecture by artist Gustav Metzger.

 

Credit

Produced by Intersections (Newcastle University) and The Arts Catalyst

 

 

The Cassini spacecraft monitors the myriad cloud forms that drift in

Saturn's atmosphere, helping scientists gain a better understanding of how

energy is transported around, and from within, the planet.

  

This view looks toward the unilluminated side of the rings from about 23

degrees above the ringplane. Saturn's shadow hides the rings at top.

  

The image was taken with the Cassini spacecraft wide-angle camera on Feb.

25, 2008 using a spectral filter sensitive to wavelengths of infrared

light centered at 752 nanometers. The view was obtained at a distance of

approximately 1.6 million kilometers (1 million miles) from Saturn. Image

scale is 94 kilometers (58 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

 

credit: NASA/JPL/Space Science Institute

 

Undulations mark both sides of the path of Saturn's moon Daphnis through

the A ring.

  

Daphnis may be small at only 8 kilometers (5 miles) across, but the moon's

gravity is great enough, and the Keeler gap in which it resides is narrow

enough, so that the perturbed particles create the wavelike patterns seen

here.

  

This view looks toward the unilluminated side of the rings from about 47

degrees above the ringplane. The image was taken in visible light with the

Cassini spacecraft narrow-angle camera on Feb. 21, 2009. The view was

acquired at a distance of approximately 1.1 million kilometers (684,000

miles) from Daphnis and at a Sun-Daphnis-spacecraft, or phase, angle of 50

degrees. Image scale is 7 kilometers (4 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.credit: NASA/JPL/Space Science Institute

 

The Cassini spacecraft views the gauzy C ring of Saturn, with the

cloud-streaked planet providing a dramatic backdrop.

  

This view looks toward the unilluminated side of the rings from about 32

degrees above the ringplane. The image was taken in visible light with the

Cassini spacecraft narrow-angle camera on Feb. 5, 2008. The view was

obtained at a distance of approximately 1.5 million kilometers (960,000

miles) from Saturn and at a Sun-ring-spacecraft, or phase, angle of 46

degrees. Image scale is about 11 kilometers (7 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov.

The Cassini imaging team homepage is at ciclops.org.

 

credit: NASA/JPL/Space Science Institute

Saturn - July 19th taken at the same time the Cassini probe was taking images looking back at Earth.

 

step one in assembly a realistic planetary mobile for the Wee Guy's room

Jupiter and Venus having a little party. December 1st will be even more fun with the moon joining in: www.spaceweather3.com/images2008/01dec08/skymap_01dec08.g...

Owl Nebula (M97) in Ursa Major - Dual 7nm narrow-band (Optolong L-eXtreme filter) image, consisting 120 five minute exposures stacked in Deep Sky Stacker: a total of 10 hours of integrated data (H-alpha and OIII). Explore Scientific ED APO 152mm, f=1200mm, f/7.9 refractor telescope. Telescope was tracked on a Skywatcher EQ8-R-Pro Mount and guided using PHD2 software.

Also includes 30 Dark frames, 30 Flat frames and 30 Dark-Flat frames. Post processed in Photoshop. This planetary nebula is about 2600 light years from us and estimated to be about 8000 years old. It is the end of life for a low-to-medium mass star. Our Sun has a similar fate. Taken in bright Moon-light.

This lil album artwork was made using some Polaroids I took of Chicago on a foggy day. It was designed by Christopher Wiitala (Dot Com).

 

Chicago, IL

 

The Cassini spacecraft catches a hint of topography on Janus, which orbits

Saturn just outside the planet's narrow F ring.

  

This view looks toward the unilluminated side of the rings from about 12

degrees above the ringplane. Janus is 179 kilometers (111 miles) across.

  

The image was taken in visible light with the Cassini spacecraft

narrow-angle camera on April 14, 2008. The view was acquired at a

distance of approximately 1.5 million kilometers (930,000 miles) from

Janus and at a Sun-Janus-spacecraft, or phase, angle of 22 degrees. Image

scale is 9 kilometers (6 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

 

credit: NASA/JPL/Space Science Institute

hay chicas ahí también

That little splotch is a small nebula.

This project was created for the first edition of MOCarze, a contest hosted on the Discord server. I built it in August 2024.

 

The rings of Saturn glow softly as sunlight from below wends its way

through. Some of the Sun's light bounces off the rings' opposite side and

can be seen illuminating Saturn's night side southern hemisphere.

  

Such a view is only possible from the Saturn-orbiting Cassini spacecraft.

  

This view looks toward the unilluminated side of the rings from about 33

degrees above the ringplane. Shadows of the innermost rings are cast upon

the planet at upper left. The edge of Saturn's shadow cuts a straight line

across the rings near upper right.

  

The image was taken in visible light with the Cassini spacecraft

wide-angle camera on March 30, 2007 at a distance of approximately 1.9

million kilometers (1.2 million miles) from Saturn. Image scale is 117

kilometers (73 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

  

credit: NASA/JPL/Space Science Institute

 

A sliver of "ringshine" pierces the darkness of Saturn's night side.

  

This view looks toward the unilluminated side of the rings from about 58

degrees above the ringplane.

  

The ring shadows fall into darkness beyond the terminator in the north.

South of the equator, a dim glow brightens the darkened globe. This light,

called ringshine, comes from sunlight reflected off the sunward side of

the expansive rings (the opposite face of the ringplane from this

perspective). The effect is pronounced in the eclipse view PIA08329.

  

The image was taken in visible light with the Cassini spacecraft

wide-angle camera on April 19, 2008. The view was obtained at a distance

of approximately 851,000 kilometers (529,000 miles) from Saturn. Image

scale is 48 kilometers (30 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

 

credit: NASA/JPL/Space Science Institute

 

As they wheel about the planet, Saturn's sunlit rings often exhibit dark,

radial markings called spokes.

  

Spokes are seen only in the broad B ring, and can also appear bright in

certain viewing geometries (see PIA08302).

  

This view looks toward the sunlit side of the rings from about 11 degrees

below the ringplane.

  

Pandora (81 kilometers, or 50 miles across) is a speck above the rings at

left. The planet's shadow darkens the ringplane at lower right.

  

The image was taken in visible light with the Cassini spacecraft

wide-angle camera on June 3, 2008. The view was acquired at a distance of

approximately 1 million kilometers (636,000 miles) from Saturn and at a

Sun-Saturn-spacecraft, or phase, angle of 19 degrees. Image scale is 61

kilometers (38 miles) per pixel.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team

homepage is at ciclops.org.

 

credit: NASA/JPL/Space Science Institute

Planetary nebula in the cluster M 46.

Mark Quinn's 'Planet', on show at Chatsworth House as part of the 'Beyond Limits' exhibition with Sothebys.

Model of he planets at the Smithsonian Air and Space Museum, Washington, D.C.

  

 

Animation Ice Moon Rendezvous

   

Zooming in closer and closer, this movie chronicles Cassini's targeted

flyby of Dione, with Saturn and its lovely rings forming a dramatic

backdrop.

  

The movie begins with Cassini during its approach about 107,000 kilometers

(66,000 miles) from the icy moon. Few surface details are discernable from

this distance, but the view quickly improves. The movie jumps to a point

39,000 kilometers (24,000 miles) from Dione, with Saturn's atmosphere now

in the background and draped by threadlike ring shadows.

  

As the spacecraft gets still closer, the camera focuses on bright

fractures in the west. It becomes apparent that these braided canyons

slice through older craters. At the closest point in this approach

sequence, Cassini is about 4,000 kilometers (2,500 miles) above Dione's

surface and the image scale is 234 meters (768 feet) per pixel. For a

narrow-angle camera image taken at almost the same instant see PIA07748.

  

A dramatic shift in perspective follows, with Cassini moving past the

point of closest approach and staring at a large crater on Dione's

receding limb. Steep cliffs gleam in the sunlight as the intrepid craft

pulls away. About three and a half hours have elapsed since the first

image in the movie was taken.

  

This movie was created from clear-filter images taken during the Oct. 11,

2005, flyby of Dione. All images except the departing view were obtained

with the Cassini spacecraft wide-angle camera.

  

The Cassini-Huygens mission is a cooperative project of NASA, the European

Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,

a division of the California Institute of Technology in Pasadena, manages

the mission for NASA's Science Mission Directorate, Washington, D.C. The

Cassini orbiter and its two onboard cameras were designed, developed and

assembled at JPL. The imaging operations center is based at the Space

Science Institute in Boulder, Colo.

  

For more information about the Cassini-Huygens mission visit

saturn.jpl.nasa.gov. The Cassini imaging team homepage is at

ciclops.org.

  

credit: NASA/JPL/Space Science Institute

1 2 ••• 66 67 69 71 72 ••• 79 80